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<ri:Resource created="2008-09-21T12:10:21Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>X-ray variability of AGNs in Lockman Hole</title><shortName>J/A+A/487/475</shortName><identifier>ivo://CDS.VizieR/J/A+A/487/475</identifier><altIdentifier>doi:10.26093/cds/vizier.34870475</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Papadakis I.E.</name></creator><creator><name>Chatzopoulos E.</name></creator><creator><name>Athanasiadis D.</name></creator><creator><name>Markowitz A.,Georgantopoulos I.</name></creator><date role="Updated">2017-09-19T14:21:22Z</date><date role="Created">2008-09-21T12:10:21Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>active-galactic-nuclei</subject><subject>x-ray-sources</subject><subject>redshifted</subject><description>We present the results from a detailed X-ray variability analysis of 66 AGN in the Lockman Hole, which have optical spectroscopic identifications. We compare, quantitatively, their variability properties with the properties of local AGN, and we study the "variability - luminosity" relation as a function of redshift, and the "variability - redshift" relation in two luminosity bins. We use archival data from the last 10 XMM-Newton observations of the Lockman Hole field to extract light curves in the rest frame, 2-10keV band. We use the "normalized excess variance" to quantify the variability amplitude. Using the latest results regarding the AGN power spectral shape and its dependence on black hole mass and accretion rate, we are able to compute model "variability - luminosity" curves, which we compare with the relations we observe. When we consider all the sources in our sample, we find that their variability amplitude decreases with increasing redshift and luminosity.</description><source format="bibcode">2008A&amp;A...487..475P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/487/475</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/329/482">J/A+A/329/482 : ROSAT Deep Survey in the Lockman Hole (Hasinger+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/53/445">J/PASJ/53/445 : ASCA Deep survey in Lockman Hole Field (Ishisaki+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/393/425">J/A+A/393/425 : Spectral analysis of Lockman Hole (Mainieri+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/398/901">J/A+A/398/901 : VLA survey at 6 cm in the Lockman Hole (Ciliegi+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/413/843">J/A+A/413/843 : Far IR survey in the Lockman Hole (Kawara+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/427/23">J/A+A/427/23 : 14.3um survey in the Lockman Hole (Fadda+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/427/773">J/A+A/427/773 : ISOCAM 14.3um Deep Survey in Lockman Hole (Rodighiero+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1501">J/AJ/128/1501 : CLASXS: X-ray catalog (Yang+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/434/801">J/A+A/434/801 : X-ray sources near Lockman Hole (Zappacosta+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/444/79">J/A+A/444/79 : XMM observations of Lockman Hole brightest AGNs (Mateos+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/473/105">J/A+A/473/105 : Lockman Hole AGN variability with XMM (Mateos+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/479/283">J/A+A/479/283 : XMM observations of the Lockman Hole (Brunner+, 2008)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/487/475</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/487/475</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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